A grid of model atmospheres and synthetic spectra for white dwarfs with an effective temperature in the range 5000-7000 K

Details A grid of model atmospheres and synthetic spectra for white dwarfs with an effective temperature in the range 5000-7000 K A grid of model atmospheres and synthetic spectra for white dwarfs with an effective temperature in the range 5000-7000 K

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48...13w&link_type=abstract

(European Workshop on White Dwarfs, 2nd, Rome, Italy, Sept. 10-14, 1976.) Società Astronomica Italiana, Memorie, vol. 48, Mar. 1

Astronomy and Astrophysics

Astronomy

15

Atmospheric Models, Stellar Atmospheres, Stellar Spectra, White Dwarf Stars, Abundance, H Lines, Helium, Hydrogen Atoms, Line Spectra, Newton-Raphson Method, Spectral Resolution, Stellar Structure

Scientific paper

A grid of model atmospheres is constructed for very cool white dwarfs in
an effort to evaluate the effect of abundance changes in such stars. The
physical properties of the models are discussed in detail and attention
is given to the computed spectra.

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